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Burton (1972) has suggested that within our Galaxy the data can be interpreted as if the HI is optically thin. 15) 29 but the Doppler' broadening produced by thermal motions in the clouds gives the line a finite width. Other motions within the clouds, such as turbulence, rotation, expansion, and contraction, will also produce line broadening. In Chapter 4 the effects of streaming as a broadening mechanism are discussed. Within each cloud the atoms have a Maxwellian velocity distribution due to their thermal motions, which means that the numbers at.
And H. H. Aumann. 1970. Astrophys. 162:179. Mathewson, D. S. 1968. J. 163:147. - - - , and D. K. Milne, 1965. AustralianJ. Phys. 18:635. Merkelijn, J. , and M. M. Davis. 1967. Eull. Astron. Inst. Neth. 19:246. Mills, B. Y. 1959. Proc. U. Symposium. No. 9, New York: Academic Press, p. 431. PachoIczyk, A. G. 1970. Radio Astrophysics. San Francisco: W. H. Freeman. Pawsey, J. L. 1961. In Galactic Structure, A. Blaauw and M. Schmidt, eds. Chicago: University of Chicago Press, p. 219. Piddington, J.